The group has more than 50 galaxies (including dwarf galaxies). Its center of mass is somewhere between the Milky Way and the Andromeda galaxy. The galaxies of the Local Group cover a 10 million light-year diameter and have a binary (dumbbell) shape.[not in the source given] The group has a total mass of about (1.29 ± 0.14)×1012Ms. The group itself is part of the Virgo Supercluster (also called the Local Supercluster).
History[change | change source]
The term "Local Group" was introduced by Edwin Hubble in 1936. He describes it as "a typical small group of nebulae which is isolated in the general field". He listed the galaxies, by decreasing luminosity, as the Andromeda galaxy, the Milky Way, Triangulum galaxy, the Large Magellanic Cloud, the Small Magellanic Cloud and half-a-dozen others.
By 2003, the number of known Local Group members has increased from his initial twelve to thirty-six, by way of the discovery of almost two dozen low-luminosity galaxies.
Related pages[change | change source]
References[change | change source]
- Karachentsev I.D. & Kashibadze O.G. (2006). "Masses of the local group and of the M81 group estimated from distortions in the local velocity field". Astrophysics 49 (1): 3–18. doi:10.1007/s10511-006-0002-6.
- R.B. Tully (1982). "The Local Supercluster". Astrophysical Journal 257: 389–422. doi:10.1086/159999.
- Hubble, Edwin 1936. The realm of the nebulae, pages 124–151
- van den Bergh, Sidney (2003). "History of the Local Group". in: "The Local Group as an Astrophysical Laboratory" (Cambridge University Press)